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Relativistic Hydrodynamics for Astrophysical Accretion

Special Relativity Essentials → Relativistic Accretion Disk Models

This learning path guides astrophysics students from the foundations of special relativity and tensor calculus through the relativistic formulation of perfect fluids and conservation laws, culminating in the construction and analysis of accretion disk models. It emphasizes the physical and mathematical prerequisites necessary to understand hydrodynamics in curved spacetime.

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13 steps · 13 nodes · 3 stages

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13 steps · 3 stages. Click any step to inspect it and see it on the Path Map.

Stage 1

Foundation

5 steps

Stage 2

Core Concepts

4 steps

Stage 3

Advanced Topics

4 steps

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Foundation

Core Concepts

Advanced Topics

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